325 research outputs found
Scalar modifications to gravity from unparticle effects may be testable
Interest has focussed recently on low energy implications of a nontrivial
scale invariant sector of an effective field theory with an IR fixed point,
manifest in terms of ``unparticles'' with peculiar properties. If unparticle
stuff exists it could couple to the stress tensor and mediate a new 'fifth'
force which we call 'ungravity' arising from the exchange of unparticles
between massive particles, which in turn could modify the inverse square law.
Under the assumption of strict conformal invariance in the hidden sector down
to low energies, we compute the lowest order ungravity correction to the
Newtonian gravitational potential and find scale invariant power law
corrections of type where is an
anomalous unparticle dimension and is a characteristic length scale
where the ungravity interactions become significant. is
constrained to lie the range for a spin 2 (spin 0)
unparticle coupling to the stress tensor (and its trace) and leads to
modification of the inverse square law with dependence in the range between
, while extra dimension models with warping modify
the force law with corrections beginning with terms O for small
but exponentially suppressed for large . Thus a discrimination between extra
dimension models and ungravity is possible in future improved submillimeter
tests of gravity.Comment: 10 pages and 1 figure. Accepted for publication in Physical Review
Letters. Title changed in the revised version. Original title "Ungravity and
its possible test
LHC Phenomenology of Lowest Massive Regge Recurrences in the Randall-Sundrum Orbifold
We consider string realizations of the Randall-Sundrum effective theory for
electroweak symmetry breaking and explore the search for the lowest massive
Regge excitation of the gluon and of the extra (color singlet) gauge boson
inherent of D-brane constructions. In these curved backgrounds, the higher-spin
Regge recurrences of Standard Model fields localized near the IR brane are
warped down to close to the TeV range and hence can be produced at collider
experiments. Assuming that the theory is weakly coupled, we make use of four
gauge boson amplitudes evaluated near the first Regge pole to determine the
discovery potential of LHC. We study the inclusive dijet mass spectrum in the
central rapidity region |y_{jet}| < 1.0 for dijet masses M \geq 2.5 TeV. We
find that with an integrated luminosity of 100 fb^{-1}, the 5\sigma discovery
reach can be as high as 4.7 TeV. Observations of resonant structures in pp
\rightarrow direct \gamma + jet can provide interesting corroboration for
string physics up to 3.0 TeV. We also study the ratio of dijet mass spectra at
small and large scattering angles. We show that with the first fb^{-1} such a
ratio can probe lowest-lying Regge states for masses \sim 2.5 TeV.Comment: To be published in Physical Review
Probing Late Neutrino Mass Properties with Supernova Neutrinos
Models of late-time neutrino mass generation contain new interactions of the
cosmic background neutrinos with supernova relic neutrinos (SRNs) through
exchange of the on-shell light boson, leading to significant modification of
the differential SRN flux observed at earth. We consider Abelian U(1) model for
generating neutrino masses at low scales and we show that there is a large
parameter space in this model for which the changes induced in the flux by the
exchange of the light bosons might allow one to distinguish between neutrinos
being Majorana or Dirac particles, the type of neutrino mass hierarchy (normal
or inverted or quasi-degenerate), and could also possibly determine the
absolute values of the neutrino masses. Measurements of the presence of these
effects would be possible at the next-generation water Cerenkov detectors
enriched with Gadolinium, or a large 100 kton liquid argon detector.Comment: 29 pages latex, 15 figures included. Version to be published in Phys.
Rev. D., added discussion of signal detection for water Cerenkov and liquid
argon detectors, and discussion of non-adiabatic vs adiabatic neutrino
evolution, new figures added, references updated. Results unchange
Leptogenesis and the Small-Angle MSW Solution
The lepton asymmetry created in the out-of-equilibrium decay of a heavy
Majorana neutrino can generate the cosmological baryon asymmetry when processed
through fast anomalous electroweak reactions. In this work I examine this
process under the following assumptions: (1) maximal nu_mu/nu_tau mixing (2)
hierarchical mass spectrum m_3 >> m_2 (3) small-angle MSW solution to the solar
neutrino deficit. Working in a basis where the charged lepton and heavy
neutrino mass matrices are diagonal, I find the following bounds on the heavy
Majorana masses M_i: (a) for a symmetric Dirac neutrino mass matrix (no other
constraints), an asymmetry compatible with BBN constraints can be obtained for
min(M_2,M_3)> 10^{11} GeV; (b) if {\em any} of the Dirac matrix elements
vanishes, successful baryogenesis can be effected for a choice of min(M_2,M_3)
as low as a few times 10^{9} GeV. The latter is compatible with reheat
requirements for supersymmetric cosmologies with sub-TeV gravitino masses.Comment: 12 pages, LaTeX; version to be published in Physics Letters
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